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Temperatures at the base of the Laurentide Ice Sheet
inferred from borehole temperature data
Frédérique Rolandone, J.C. Mareschal, C. Jaupart
To cite this version:
Frédérique Rolandone, J.C. Mareschal, C. Jaupart. Temperatures at the base of the Laurentide Ice Sheet inferred from borehole temperature data. Geophysical Research Letters, American Geophysical Union, 2003, 30 (18), pp.1944. �10.1029/2003GL018046�. �hal-00067834�
Temperatures at the base of the Laurentide Ice Sheet inferred from
borehole temperature data
Fre´de´rique Rolandone,1 Jean-Claude Mareschal,2 and Claude Jaupart3
Received 24 June 2003; revised 6 August 2003; accepted 14 August 2003; published 23 September 2003.
[1] We use temperature profiles from 4 deep (>1600 m)
boreholes across Canada to determine ground surface temperature histories (GSTH’s) through and after the Last Glacial Maximum (LGM). Inversion yields the temperature history at the base of the glacier and the surface temperature evolution after the glacial retreat. The results indicate geographic differences in basal temperature history across the Ice Sheet. During the Last Glacial Maximum, temperatures at the base of the Ice Sheet were lower in eastern Canada, at the southeastern edge of the glacier, than in central Canada, southwest of the glacier center. At all sites, basal temperatures were above the melting point of ice during and after the LGM, which may explain the highly unstable character of the Ice Sheet. The GSTH’s are consistent with information on the history of the Laurentide ice sheet and provide quantitative constraints on glacier flow dynamics. INDEX TERMS: 8130 Tectonophysics: Heat generation and transport; 1827 Hydrology: Glaciology (1863); 1 6 2 0 G l o b a l C h a n g e : C l i m a t e d y n a m i c s ( 3 3 0 9 ) . Citation: Rolandone, F., J.-C. Mareschal, and C. Jaupart, Temperatures at the base of the Laurentide Ice Sheet inferred from borehole temperature data, Geophys. Res. Lett., 30(18), 1944, doi:10.1029/2003GL018046, 2003.
1. Introduction
[2] Modeling the dynamics of glacial growth and retreat
requires knowledge of the boundary conditions at the base of the ice sheet, which have a strong impact on basal temperature [Huybrechts, 1986; Licciardi et al., 1988; Marshall et al., 2000]. Such models are of special impor-tance for understanding catastrophic meltwater discharges from the Laurentide Ice Sheet that may have been respon-sible for climatic instability and for Heinrich events [Payne, 1995; Clark et al., 2001]. The lack of subglacial paleotem-perature records has led to searches for proxies [Kleman and Hattestrand, 1999].
[3] Temporal changes in ground surface temperature
propagate in the solid rock basement and are recorded as perturbation of the steady-state temperature profile. It is therefore possible to determine the ground surface temper-ature history by inversion of vertical tempertemper-ature profiles measured in boreholes [Vasseur et al., 1983; Shen and Beck, 1992; Mareschal and Beltrami, 1992]. Several
studies have shown that borehole data lead to reliable inferences on climatic changes over the last millenium [Lewis, 1992]. Here, we use deep boreholes to go further back in time. In order to detect the cold period of the last glacial maximum (LGM) and subsequent warming, we need temperature profiles deeper than 1,500 m. So far, two studies of temperature profiles have yielded informa-tion on the thermal condiinforma-tions at the base of the ice sheet in Canada. Sass et al. [1971] used a deep borehole (2865 m) near Flin-Flon, Manitoba, to show that, during the LGM, surface temperature was less than 5K colder than present. They did not invert the temperature profile for detailed reconstruction of the GSTH. Mareschal et al. [2000a] used a deep (1800 m) hole near Sept-Iles, Quebec, to show that ground surface temperature during the LGM was 10 K colder than present. A very recent statistical study of heat flow variations in deep boreholes in the Fennoscandian Shield and the Russian platform suggests that, during the LGM, temperatures were 8 K colder than at present in ice free regions but that there was less cooling in ice covered regions [Kukkonen and Jo˜eleht, 2003]. To study conditions beneath the Laurentide ice sheet, we revisit the Sept-Iles and Flin-Flon profiles and add data from 2 other deep boreholes in central Canada: one (1725 m) in Balmertown, northwestern Ontario, and one (1610 m) near Thompson, Manitoba. The location of these sites in relation to the Laurentian glacier is shown in Figure 1.
2. Borehole Temperature Data Used in This Study
[4] For analysis, the critical assumption is that of purely
vertical conductive heat transport in the rock underlying the ice sheet. Local perturbations due to groundwater flow in fractures or heat refraction effects across media of contrasting thermal properties must therefore be avoided. The data for this study were collected during extensive heat flow surveys of the Canadian Shield [Mareschal et al., 2000b; Rolandone et al., 2002, 2003]. Because several boreholes were logged at each site, thermal con-ditions in the vicinity of these deep boreholes are well controlled.
[5] Figure 2 shows the thermal conductivity and the
variation in heat flow with depth for the profiles. The 1800 m Sept-Iles borehole was drilled in a massive gabbro intrusion without conductivity variation with depth. While the lithology may be more complicated at the three other sites, the only site with systematic conductivity variation is Flin-Flon where the conductivity decreases below 1800 m [Sass et al., 1971], which was accounted for when deter-mining the heat flow profile. For the other three sites, we
1Berkeley Seismological Laboratory, UC Berkeley, USA. 2
GEOTOP-UQAM-McGill, Centre de Recherche en Ge´ochimie et en Ge´odynamique, Universite´ du Que´bec a` Montre´al, Canada.
3
Institut de Physique du Globe de Paris, France.
Copyright 2003 by the American Geophysical Union. 0094-8276/03/2003GL018046
have used the average thermal conductivity to determine the heat flow profile.
3. Inversion Results
[6] The temperature at depth z in a borehole is written as:
T zð Þ ¼ Tref þ Qref
Z z 0
dz0
k zð Þ0 þ Ttð Þz ð1Þ
where Trefis the reference ground surface temperature in the
absence of perturbations, Qrefthe steady-state heat flux from
depth, k(z) thermal conductivity and Tt(z) the
time-dependent temperature field due to ground surface tem-perature changes. Heat production can be included in the analysis [Clauser and Mareschal, 1995] but it was found to be small at all the boreholes used and thus neglected for this study. For each site, we have inverted the temperature profile to determine the GSTH. The ground temperature history is approximated by a function that varies in a stepwise manner between intervals within which it remains constant. Because we are considering a long history, we
have used a logarithmic distribution for the duration of the time intervals that become larger as time increases. This parameterization yields a system of equations for the temperatures during each interval and for the reference heat flow and surface temperature. This linear system of equations is ill-conditioned. Following Mareschal and Beltrami [1992], we have stabilized its solution with an inversion algorithm based on the singular value decom-position [Lanczos, 1961]. The instability is avoided by replacing the inverse of the singular values 1/l by l/(l2+ ) where the value of e depends on the noise level. This stabilization is obtained by decreasing the resolution: in practice, for an event to be resolved, its duration must be >1/4 the time it occurred [Beltrami and Mareschal, 1995]. In order to have comparable resolution, we have used the same value = 0.08 for all profiles. Monte-Carlo inversions [Mareschal et al., 2000a] have also been applied with similar results and suggest that the uncertainty in the paleotemperature results is about ±1 K.
[7] Table 1 lists the relevant parameters including the
minimum ground surface temperature during the LGM, Tmin, and the time interval when it was reached. The ground
Figure 1. Ice thickness of the Laurentide glacier at 21 ka. Ice thickness model ICE-4G from Peltier [2002]. Red triangles mark the location of the deep drillholes used in this study.
surface temperature histories of the four sites are shown on Figure 3.
[8] The Flin-Flon drill hole is deeper and should give
better constraints than the others for events occurring between 10 to 100 kyears B.P. Three profiles show the same temperature trends, with a minimum at ca. 10,000 – 20,000 years, followed by a warming episode peaking at ca. 3,000 – 4,000 years and one cooling episode peaking a few hundred years ago. The amplitudes, however, are different. The total amplitude of the ground surface temperature variation at Sept-Iles is more than twice that at Flin-Flon. The amplitude is small at Thompson and Balmertown. There is not much difference in model resolution between Sept-Iles, Thompson, and Balmertown. The resolution dif-ference might explain why the amplitudes of the Balmer-town and Thompson GSTH’s are lower than at Flin-Flon, but cannot account for the amplitude difference between Sept-Iles and Flin-Flon. If anything, Sept-Iles might have an even larger amplitude than indicated in Figure 3, as shown
by the slightly lower LGM temperature estimates deduced from a Monte-Carlo inversion [Mareschal et al., 2000a].
[9] The minimum temperatures were reached at different
times around the LGM (21 ka) when the ice thickness was maximum. A warming episode is recorded at the 4 sites which may be attributed to ice retreat. The warming at Sept-Iles seems to have started between 20 and 15,000 years B.P., while it started betwen 10 and 8,000 years B.P. at Flin-Flon. Despite the low amplitude of temperature variations in Balmertown and Thompson, the GSTH’s at these two sites also suggests that ground surface temperature warming started later than at Sept-Iles. These GST histories are consistent with information on the history of the Laurentide ice sheet. Reconstructions of the Laurentide Ice Sheet indicate that the Sept-Iles and Flin-Flon sites became free of ice at ca. 14,000 and 11,500 years B.P. respectively [Licciardi et al., 1998; Dyke and Prest, 1982]. Massive meltwater discharge from the mid-continent lobes of the Laurentide Ice Sheet is recorded between 9,000 and 8,500 years in Lake Winnipeg and Lake Michigan sediments [Moore et al., 2000].
4. Discussion
[10] Although much colder temperatures at the base of
the ice sheet are predicted by some models of ice dynamics [Marshall and Clark, 2002], it does not come as a surprise that there were spatial variations in temperature at the base of the Laurentide ice sheet. Present bedrock temperatures measured beneath the central part of the Greenland ice sheet are8 and 13C [Dahl-Jensen et al., 1998]. Temperatures are higher in areas where basal melts have been detected [Fahnestock et al., 2001]. In Antarctica, temperatures near 0C were measured at the base of the fast moving ice stream Figure 2. Thermal conductivity, and heat flow for the four
deep temperature depth profiles used in this study. Conductivity measurements for Sept-Iles, Balmertown, and Thompson were made on core samples with the divided bar. Conductivity measurements at Flin-Flon were made with the needle probe and the conductivity profile represents the average from many measurements.
Figure 3. Ground surface temperature history inverted from borehole temperature profiles for the period 100 ka to present. Temperature shifted as indicated. The same value of the regularization parameter = 0.08 was used for the four inversions.
Table 1. Temperature Depth Profiles Used in This Study
Site Latitude deg min Longitude deg min Depth m TrefC QrefmWm2 TminC Time kyears BP
Sept-Iles (QC) 50130N 66380W 1810 m 2.1 34 1.5 20 – 30 Balmertown (ON) 51020N 93430W 1725 m 3.5 35 2.1 8 – 15 Flin-Flon (SK) 54930N 102000W 2865 m 3.4 42 0.4 10 – 20 Pipe Mine, Thompson (MB) 55290N 98080W 1610 m 2.4 51 0.4 8 – 12
The table gives the geographic location, the depth of the borehole, the reference ground surface temperature, the reference heat flow, the minimum temperature recorded during the last glaciation, and the time when it occurred.
at holes B, C, and D [Engelhardt and Kamb, 1993; Parizek et al., 2002]. Temperature at the base of the glacier depends much on the accumulation and flow of ice as well as on the geothermal heat flux. Sept-Iles is closer to the edge of the ice-sheet than the other sites and more rapid flow of ice may have resulted in colder conditions at the base. Also, Sept-Iles has the lowest heat flux of all these sites (51 mWm2at Thompson vs 34 mWm2 at Sept-Iles), which may also partly account for the GSTH difference between these two sites. Such control of heat flow on glacier dynamics is suggested by the study of Tarasov and Peltier [2003].
[11] These results have implications for Ice Sheet models
which depend on several poorly constrained parameters and processes, such as climatic changes, geographical distribu-tion of snow fall and basal mechanical boundary condidistribu-tions. For example, depending on the behaviour of basal till and ice bed, the Laurentide Ice Sheet may have developed multiple ice domes [Licciardi et al., 1998]. As emphasized by Marshall et al. [2000], there are large differences in the predicted basal temperatures between models. Our results may thus provide useful constraints on the boundary con-ditions. Our data show that, along its southern margin, the Laurentide Ice Sheet was not frozen to the bed, implying basal sliding. It is well-established that such conditions lead to an unstable ice sheet with limit cycles in the basal thermal regime and sliding velocity [Payne, 1995].
[12] Acknowledgments. Shawn Marshall, Dick Peltier, and John Sass provided much useful information. We are grateful to an anonymous reviewer for drawing our attention to the Antarctic ice stream temperature data. This research was supported by LITHOPROBE, NSERC (Canada) and INSU (CNRS, France).
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F. Rolandone, Seismological Laboratory, UC Berkeley, 215 McCone Hall, Berkeley 94720,CA, USA. (frede@seismo.berkeley.edu)
J.-C. Mareschal, Geotop, UQAM, C.P. 8888,Succ. Centre-Ville, Montre´al, H3C 3P8, Canada. (jcm@olympus.geotop.uqam.ca)
C. Jaupart, Institut de Physique du Globe de Paris, 4 Place Jussieu, 75252 Paris cedex 05, France. (cj@ccr.jussieu.fr)